Hubble Space TelescopeImaging of the CFRS and LDSS Redshift Surveys. I. Morphological Properties-Reference-Cited by-同舟云学术

Hubble Space TelescopeImaging of the CFRS and LDSS Redshift Surveys. I. Morphological Properties

Published:1998-05-20 Issue:1 Volume:499 Page:112-133
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Brinchmann Jarle,Abraham Roberto,Schade David,Tresse Laurence,Ellis Richard S.,Lilly Simon,Le Fevre Olivier,Glazebrook Karl,Hammer Francois,Colless Matthew,Crampton David,Broadhurst Tom

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/499/i=1/a=112/pdf

Reference42 articles.

1. Abraham, B., Freedman, W. & Madore, B. 1997, in Proc. 36th Herstmonceux Conf., HST and the High-Redshift Universe, ed. N. Tanvir, A. Aragon-Salamanca, & J. V. Wall (Singapore: World Scientific)

2. Galaxy morphology to I=25 mag in the Hubble Deep Field

3. The morphologies of distant galaxies. 1: an automated classification system

4. The Morphologies of Distant Galaxies. II. Classifications from the Hubble Space Telescope Medium Deep Survey

5. Faint galaxy counts as a function of morphological type in a hierarchical merger model

Cited by 200 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A morphological analysis of the galaxy cluster XLSSC 122 at z = 1.98;Monthly Notices of the Royal Astronomical Society;2024-08-15

2. A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at 0 ≲ z ≲ 5;Astronomy & Astrophysics;2024-07

3. Sp1149. I. Constraints on the Balmer L–σ Relation for H ii Regions in a Spiral Galaxy at Redshift z = 1.49 Strongly Lensed by the MACS J1149 Cluster;The Astrophysical Journal;2024-06-28

4. Properties of the brightest young stellar clumps in extremely lensed galaxies at redshifts 4 to 5;Monthly Notices of the Royal Astronomical Society;2024-02-28

5. Bulgeless disks, dark galaxies, inverted color gradients, and other expected phenomena at higher z;Astronomy & Astrophysics;2023-04-27